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Earth in Space

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EARTH IN SPACE









Key Concepts

How does Earth move in space?

What causes the cycle of seasons on

Earth?

Key Terms



 Astronomy  Orbit

 Axis  Calendar

 Rotation  Solstice

 Revolution  Equinox

How Earth Moves

• Astronomy –the study of the moon, stars and other

objects in space

• Earth moves through space in two major ways:

rotation and revolution

• Rotation- the spinning of Earth on its axis

• Axis – imaginary line through Earth’s center and North and

South poles

• Rotation causes day and night

• Takes 24 hours for one rotation

• Revolution- movement of one object around

another

• One complete revolution of Earth around the sun is

a year

• Earth follows a slightly elliptical orbit around sun

Rotation vs Revolution

Checkup



 How many rotations of Earth take

place in one revolution around the

sun?

Calendars

• A Calendar is system of organizing the

time that defines the beginning, length

and divisions of a year

• People of many cultures have added to our idea

of a calendar

• Egyptians determined that there are 365 days in

a year

• Many people followed moon cycles – there are

about 29 ½ days in a moon cycle or month

• Problem = 12 moon cycles of 30 days only adds

up to 354 days.

Calendar

• Romans borrowed Egyptian calendar of

365 days

• Problem: It actually takes the Earth 365 ¼ days to

complete one revolution. The Romans added 1 day

every 4 years. The 4th year is known as a leap year

• Problem: Roman calendar still off by 11 min. Over

the centuries the minutes added up and by 1500’s

the beginning of spring was coming 10 days early

• Pope Gregory XIII dropped 10 days from the

Calendar to correct. He also made other minor

changes.

• This is the calendar we use today

Check up



 What is a leap year?







 Explain why it was difficult for ancient

peoples to develop workable calendars

The Seasons on

Earth

 Temperate places on Earth have 4 seasons:

 Winter, spring, summer, fall

 How sunlight hits the Earth affects how warm

an area is.

 Sunlight hits more directly and a smaller area

at the equator so it is warmer

 Sunlight hits at an angle and over a greater

area at the poles so it is colder

Earth’s Tilted Axis

• Earth has seasons because its axis

is tilted as it revolves around the

sun. (23.5° from vertical)

• As Earth revolved around the sun, the north

end is tilted towards the sun for half of the

year and tilted away the other half

• Summer and winter are caused by the Earth’s

tilt not by changes in Earth’s distance from

the sun

• Earth is actually farthest from the sun during

the northern hemisphere’s summer

Earth in June



 North end of Earth’s axis

is tilted toward the sun

 Sun is higher in the sky and there are more hours of

sunlight

 Sun’s rays are more direct

 It is summer in Northern Hemisphere

 South end of Earth’s axis is tilted away

 Sun is low in the sky, days are shorter than nights

 Sun’s rays are more slanted

 It is winter in southern hemisphere

Earth in December



 Southern Hemisphere receives most direct

sunlight – summer

 Northern Hemisphere receives slanted rays -

winter

Solstices

 Solstice – when sun is farthest north or south of

the equator

 Day when the sun is farthest north of the

equator = about June 21 = Summer Solstice in

the Northern Hemisphere and Winter Solstice in

Southern Hemisphere

 Day when the sun is farthest south of the

equator = about December 21= Winter Solstice

in Northern Hemisphere and Summer Solstice in

Southern Hemisphere

Equinoxes



 Halfway between the solstices, neither

hemisphere is tilted toward or away from sun

 Noon is directly overhead at the equator

 Day and night are equal lengths - about 12

hours each

 Occurs twice a year around March 21(Vernal

or spring equinox) and September 21

(autumnal equinox)

Solstices and

Equinoxes

Check up



 If Earth’s axis were not tilted,

what would happen to the length

of days over the course of a year?



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